D. Elbaz

Publication List Details

Period

1994 - 2009

Number

103

Co-Authors

Very High Gas Fractions and Extended Gas Reservoirs in z=1.5 Disk Galaxies (2009)

Daddi, E., Bournaud, F., Walter, F., Dannerbauer, H., Carilli, C., Dickinson, M., ...

We present evidence for very high gas fractions and extended molecular gas reservoirs in normal, near-infrared selected (BzK) galaxies at z~1.5, based on multi-configuration CO[2-1] observations...

Quasar induced galaxy formation: a new paradigm ? (2009)

Elbaz, D., Jahnke, K., Pantin, E., Borgne, D. Le, Letawe, G.

We discuss observational evidence that quasars play a key role in the formation of galaxies starting from the detailed study of the quasar HE0450-2958 and extending the discussion to a series of...

Low, Milky-Way like, Molecular Gas Excitation of Massive Disk Galaxies at z~1.5 (2009)

Dannerbauer, H., Daddi, E., Riechers, D. A., Walter, F., Carilli, C. L., Dickinson, M., ...

We present evidence for Milky-Way-like, low-excitation molecular gas reservoirs in near-IR selected massive galaxies at z~1.5, based on IRAM Plateau de Bure Interferometer CO[3-2] and NRAO Very Large...

A CO emission line from the optical and near-IR undetected submillimeter galaxy GN10 (2009)

Daddi, E., Dannerbauer, H., Krips, M., Walter, F., Dickinson, M., Elbaz, D., ...

We report the detection of a CO emission line from the submillimiter galaxy (SMG) GN10 in the GOODS-N field. GN10 lacks any counterpart in extremely deep optical and near-IR imaging obtained with the...

The 0.4 < z < 1.3 star formation history of the Universe as viewed in the far-infrared (2009)

Magnelli, B., Elbaz, D., Chary, R. R, Dickinson, M., Borgne, D. Le, Frayer, D. T., ...

[Abridged] We use the deepest existing mid- and far-infrared observations (reaching ~3 mJy at 70 um) obtained with Spitzer in the GOODS and FIDEL fields to derive the evolution of the rest-frame 15...

Reliable Identification of Compton-thick Quasars at z ≈ 2: Spitzer Mid-Infrared Spectroscopy of HDF-oMD49 (2008)

Alexander, D. M., Pope, A., Bauer, F. E., Brandt, W. N., Daddi, E., ...

Many models that seek to explain the origin of the unresolved X-ray background predict that Compton-thick active galactic nuclei (AGNs) are ubiquitous at high redshift. However, few distant...

Two bright submillimeter galaxies in a z=4.05 proto-cluster in GOODS-North, and accurate radio-infrared photometric redshifts (2008)

Daddi, E., Dannerbauer, H., Stern, D., Dickinson, M., Morrison, G., Elbaz, D., ...

We present the serendipitous discovery of z=4.05 molecular gas CO emission lines with the IRAM Plateau de Bure interferometer coincident with GN20 and GN20.2, two luminous submillimeter galaxies...

IRAC excess in distant star-forming galaxies: tentative evidence for the 3.3 μm polycyclic aromatic hydrocarbon feature? (2008)

Magnelli, B., Chary, R. R., Pope, A., Elbaz, D., Morrison, G., Dickinson, M.

We present evidence for the existence of an IRAC excess in the spectral energy distribution (SED) of five galaxies at 0.6 < z < 0.9 and one galaxy at z = 1.7. These six galaxies, located in the Great...

Observations and modelling of a clumpy galaxy at z=1.6: Spectroscopic clues to the origin and evolution of chain galaxies (2008)

Bournaud, F., Daddi, E., Elmegreen, B. G., Elmegreen, D. M., Nesvadba, N., Vanzella, E., ...

We investigate the properties of a clump-cluster galaxy at redshift 1.57. The morphology of this galaxy is dominated by eight star-forming clumps in optical observations, and has photometric...

Reliable Identification of Compton-thick Quasars at z~2: Spitzer Mid-IR spectroscopy of HDF-oMD49 (2008)

Alexander, D. M., Chary, R. R., Pope, A., Bauer, F. E., Brandt, W. N., Daddi, E., ...

Many models that seek to explain the origin of the unresolved X-ray background predict that Compton-thick Active Galactic Nuclei (AGNs) are ubiquitious at high redshift. However, few distant...

Vigorous star formation with low efficiency in massive disk galaxies at z = 1.5 (2008)

Daddi, E., Dannerbauer, H., Elbaz, D., Dickinson, M., Morrison, G., Stern, D., ...

We present the first detection of molecular gas cooling CO emission lines from ordinary massive galaxies at z=1.5. Two sources were observed with the IRAM Plateau de Bure Interferometer, selected to...

Vigorous star formation with low efficiency in massive disk galaxies at z=1.5 (2007)

Daddi, E., Dannerbauer, H., Elbaz, D., Dickinson, M., Morrison, G., Stern, D., ...

We present the first detection of molecular gas cooling CO emission lines from ordinary massive galaxies at z=1.5. Two sources were observed with the IRAM Plateau de Bure Interferometer, selected to...

Deep Surveys And Cosmology (2007)

S. J. Oliver, Oliver Sergeant, P. Goldschmidt, R. G. Mann, M. Rowan-robinson, N. Eaton, ...

Introduction Surveys with ISO (Kessler et al 1996), in particular with the CAM (Cesarsky et al 1996) and PHOT (Lemke et al 1996) instruments, will greatly extend our understanding of extra-galactic...

Iso Mid-Infrared Observations Of Abell 370 (2007)

Metcalfe Altieri Aussel, L. Metcalfe, B. Altieri, H. Aussel, A. Biviano, B. Mc Breen, ...

We report on the mid-IR imaging at 7 and 10 ¯m of the galaxy cluster Abell 370, obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of an ongoing program...

Ultimate Sensitivity With Isocam (2007)

Altieri Metcalfe And, B. Altieri, L. Metcalfe, J. Blommaert, D. Elbaz, ...

. We discuss the instrumental factors which constrain the sensitivity limits of the mid-infrared camera (ISOCAM) of ESA's Infrared Space Observatory (ISO). The observing strategy judged to be...

A Deep And Ultra-Deep Isocam Cosmological Survey Through Gravitationally Lensing Clusters Of Galaxies (2007)

L. Metcalfe, B. Altieri, B. McBreen, J-p. Kneib, M. Delaney, A. Biviano, ...

We present imaging results and source counts from an ISOCAM deep and ultra-deep cosmological survey through gravitationally lensing clusters of galaxies at 7¯m and 15¯m. A total area of about 53...

Multiwavelength Study of Massive Galaxies at z ~ 2. II. Widespread Compton-thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and Bulges (2007)

Daddi, E., Alexander, D. M., Dickinson, M., Gilli, R., Renzini, A., Elbaz, D., ...

Approximately 20%-30% of 1.4 ≾ z ≾ 2.5 galaxies with K_(Vega) < 22 detected with Spitzer MIPS at 24 μm show excess mid-IR emission relative to that expected based on the rates of star formation...

The spatial clustering of mid-IR selected star forming galaxies at z ~ 1 in the GOODS fields (2007)

Gilli, R., Daddi, E., Chary, R., Dickinson, M., Elbaz, D., Giavalisco, M., ...

We present the first spatial clustering measurements of z~1, 24um-selected, star forming galaxies in the Great Observatories Origins Deep Survey (GOODS). The sample under investigation includes 495...

Far-Infrared Characterization of an Ultraluminous Starburst Associated with a Massively Accreting Black Hole at z = 1.15 (2007)

Le Floc'h, E., Willmer, C. N. A., Noeske, K., Konidaris, N. P., Laird, E. S., Koo, D. C., ...

As part of the All-Wavelength Extended Groth Strip International Survey (AEGIS), we describe the panchromatic characterization of an X-ray–luminous active galactic nucleus (AGN) in a merging galaxy...

The reversal of the star formation-density relation in the distant universe (2007)

Elbaz, D., Daddi, E., Borgne, D. Le, Dickinson, M., Alexander, D. M., Chary, R-R, ...

We study the relationship between the local environment of galaxies and their star formation rate (SFR) in the Great Observatories Origins Deep Survey, GOODS, at z~1, from ultradeep imaging at 24...

531 new spectroscopic redshifts from the CDFS and a test on the cosmological relevance of the GOODS-South field (2007)

Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...

(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ

New spectroscopic redshifts from the CDFS and a test of the cosmological relevance of the GOODS-South field (2007)

Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...

Context: .This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to a redshift of one. Intermediate mass galaxies (MJ

Multiwavelength study of massive galaxies at z~2. II. Widespread compton-thick active galactic nuclei and the concurrent growth of black holes and bulges (2007)

Daddi, E., Alexander, D. M., Dickinson, M., Gilli, R., Renzini, A., Elbaz, D., ...

Approximately 20%-30% of 1.4~1024 cm-2 and an average, unobscured X-ray luminosity L2-8keV~(1-4)×1043 ergs s-1. Their sky density (~3200 deg-2) and space density (~2.6×10-4 Mpc-3) are twice those...

531 new spectroscopic redshifts from the CDFS and a test on the cosmological relevance of the GOODS-South field (2006)

Ravikumar, C. D., Puech, M., Flores, H., Proust, D., Hammer, F., Lehnert, M., ...

(Abbrev.) This paper prepares a series of papers analysing the Intermediate MAss Galaxy Evolution Sequence (IMAGES) up to z=1. Intermediate mass galaxies (MJ

Far-infrared characterization of an ultra-luminous starburst associated with a massively-accreting black hole at z=1.15 (2006)

Floc'h, E. Le, Willmer, C. N. A., Noeske, K., Konidaris, N. P., Laird, E. S., Koo, D. C., ...

As part of the "All Wavelength Extended Groth Strip International Survey" (AEGIS), we describe the panchromatic characterization of an X-ray luminous active galactic nucleus (AGN) in a merging galaxy...

Report by the ESA-ESO Working Group on "The Herschel-ALMA Synergies" (2006)

Wilson, T. L., Elbaz, D.

The Herschel Satellite and the Atacama Large Millimeter Array (ALMA) are two very large sub-mm and far infrared (FIR) astronomy projects that are expected to come into operation in this decade. This...

Spitzer 70 Micron Source Counts in GOODS-North (2006)

Frayer, D. T., Huynh, M. T., Chary, R., Dickinson, M., Elbaz, D., Fadda, D., ...

We present ultradeep Spitzer 70 μm observations of GOODS-North (Great Observatories Origins Deep Survey). For the first time, the turnover in the 70 μm Euclidean-normalized differential source...

Spitzer 70-micron Source Counts in GOODS-North (2006)

Frayer, D. T., Huynh, M. T., Chary, R., Dickinson, M., Elbaz, D., Fadda, D., ...

We present ultra-deep Spitzer 70-micron observations of GOODS-North. For the first time, the turn-over in the 70-micron Euclidean-normalized differential source counts is observed. We derive source...

The star formation history of luminous infrared galaxies (2006)

Marcillac, D., Elbaz, D., Charlot, S., Liang, Y. C., Hammer, F., Flores, H., ...

We constrain the past star formation histories of a sample of 25 distant (z~0.7) luminous infrared galaxies (LIRGs) detected with the mid infrared cameras ISOCAM and MIPS onboard the ISO and Spitzer...

Mid infrared properties of distant infrared luminous galaxies (2006)

Marcillac, D, Elbaz, D., Chary, R. R., Dickinson, M., Galliano, F., Morrison, G.

We present evidence that the mid infrared (MIR) is a good tracer of the total infrared luminosity, L(IR), and star formation rate (SFR), of galaxies up to z 1.3. We use deep MIR images from the...

The star formation history of luminous infrared galaxies (2006)

Marcillac, D., Elbaz, D., Charlot, S., Liang, Y. C., Hammer, F., Flores, H., ...

Aims.We constrain the past star formation histories of a sample of 25 distant (bar{z}˜ 0.7) luminous infrared galaxies (LIRGs) detected with the mid infrared cameras ISOCAM and MIPS onboard the ISO...

Spitzer Observations of Massive Red Galaxies at High Redshift (2005)

Papovich, Casey, Moustakas, L. A., Dickinson, M., Floc'h, E. Le, Rieke, G. H., Daddi, E., ...

We investigate the properties of massive galaxies at z=1-3.5 using HST observations, ground-based near-IR imaging, and Spitzer Space Telescope observations at 3-24 micron. We identify 153 distant red...

Multiwavelength Observations of one Galaxy in Marano Field (2005)

Liang, Y. C., Hammer, F., Flores, H., Elbaz, D., Deng, L. C., Assemat, F., ...

We report the multiwavelength observations of one intermediate redshift (z=0.3884) galaxy in the Marano Field. These data include ISOCAM middle infrared, VLT/FORS2 spectroscopic and photometric data,...

Deep Galaxy survey at 6.75 micron with the ISO satellite (2005)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

Observational evidence for the presence of PAHs in distant Luminous Infrared Galaxies using ISO and Spitzer (2005)

Elbaz, D., Floc'h, E. Le, Dole, H., Marcillac, D.

We present ISOCAM 15 micron and MIPS 24 micron photometry of a sample of 16 distant Luminous Infrared Galaxies (LIRGs) characterized by a median luminosity L(IR) 2x10^11 Lsol and redshift z = 0.7...

The Luminosity and Metallicity Relation of distant luminous infrared galaxies (2005)

Liang, Y. C., Hammer, F., Flores, H., Elbaz, D., Marcillac, D., Deng, L., ...

Oxygen abundances [12+log(O/H)] in the interstellar medium of a large sample of distant (z>0.4) luminous infrared galaxies (LIRGs) were estimated from their extinction corrected emission-line ratios,...

Did most present-day spirals form during the last 8 Gyr? A formation history with violent episodes revealed by panchromatic observations (2005)

Hammer, F., Flores, H., Elbaz, D., Zheng, X. Z., Liang, Y. C., Cesarsky, C.

Studies of distant galaxies have shown that ellipticals and large spirals (Schade et al. \cite{Schade99}, ApJ, 525, 31; Lilly et al. \cite{Lilly98}, ApJ, 500, 75) were already in place 8 Gyr ago,...

Did most present-day spirals form during the last 8 Gyrs? A formation history with violent episodes revealed by panchromatic observations (2004)

Hammer, F., Flores, H., Elbaz, D., Zheng, X. Z., Liang, Y. C., Cesarsky, C.

(abridged) Studies of distant galaxies have shown that ellipticals and large spirals were already in place 8 Gyr ago, leading to a very modest recent star formation in intermediate mass galaxies....

ISOCAM observations in the Lockman Hole - II The 14.3 micron deep survey: data reduction, catalogue and source counts (2004)

Rodighiero, G., Lari, C., Fadda, D., Franceschini, A., Elbaz, D., Cesarsky, C.

We present a new analysis of the ISOCAM 14.3 micron deep survey in a 20x20 square arcmins area in the Lockman Hole. This survey is intermediate between the ultra-deep surveys and the shallow surveys...

The Nature of Faint 24 micron Sources Seen in Spitzer Observations of ELAIS-N1 (2004)

Chary, R., Casertano, S., Dickinson, M. E., Ferguson, H. C., Eisenhardt, P. R. M., Elbaz, D., ...

The Spitzer Space Telescope has undertaken the deepest ever observations of the 24 micron sky in the ELAIS-N1 field as part of GOODS Science Verification observations. We present the shape of the 24...

The Luminosity-Metallicity Relation of distant luminous infrared galaxies (2004)

Liang, Y. C., Hammer, F., Flores, H., Elbaz, D., Marcillac, D., Cesarsky, C. J.

One hundred and five 15mu selected objects in three ISO deep survey fields (CFRS 3h, UDSR and UDSF) are studied on the basis of the high quality optical spectra with resolution R>1000 from VLT/FORS2....

The European Large-Area ISO Survey (ELAIS): the final band-merged catalogue (2004)

Rowan-Robinson, M., Lari, C., Perez-Fournon, I., Gonzalez-Solares, E. A., La Franca, F., Vaccari, M., ...

We present the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175 ‚‚mu;m, and the associated data at U, g', r', i', Z, J, H, K and 20 cm. The origin of the...

ELAIS: final band-merged catalogue (2004)

Rowan-Robinson, M., Lari, C., Perez-Fournon, I., Gonzalez-Solares, E. A., Franca, F. L., Vaccari, M., ...

The catalog represents the final band-merged European Large-Area ISO Survey (ELAIS) Catalogue at 6.7, 15, 90 and 175{mu}m, and the associated data at U, g', r', i', Z, J, H, K and 20cm. Details about...

Star formation rates of distant luminous infrared galaxies derived from Halpha and IR luminosities (2003)

Flores, H., Hammer, F., Elbaz, D., Cesarsky, C. J., Liang, Y. C., Fadda, D., ...

We present a study of the star formation rate (SFR) for a sample of 16 distant galaxies detected by ISOCAM at 15um in the CFRS0300+00 and CFRS1400+52 fields. Their high quality and intermediate...

An ISOCAM survey through gravitationally lensing galaxy clusters (2003)

Metcalfe, L., McBreen, B., Altieri, B., Biviano, A., Delaney, M., ...

ISOCAM was used to perform a deep survey through three gravitationally lensing clusters of galaxies. Nearly seventy sq. arcmin were covered over the clusters A370, A2218 and A2390. We present maps...

Infrared spectroscopy of faint 15 micron sources in the Hubble Deep Field South: first hints at the properties of the sources of the IR background (2003)

Franceschini, A., Berta, S., Rigopoulou, D., Aussel, H., Cesarsky, C. J., Elbaz, D., ...

We present a spectroscopic analysis of 21 galaxies with z=0.2-1.5 drawn from a 25 sq. arcmin ultra-deep 15 micron ISOCAM survey centered in the HDFS. VLT/ISAAC spectra are reported for 18 sources,...

A multiwavelength approach to the SFR estimation in galaxies at intermediate redshifts (2002)

Cardiel, N., Elbaz, D., Schiavon, R. P., Willmer, C. N. A., Koo, D. C., Phillips, A. C., ...

We use a sample of 7 starburst galaxies at intermediate redshifts (z ~ 0.4 and z ~ 0.8) with observations ranging from the observed ultraviolet to 1.4 GHz, to compare the star formation rate (SFR)...

An unusual iron Lo-BAL quasar detected by ISOCAM (2002)

Hall, P. B., Fadda, D., Chanial, P., Elbaz, D., Monaco, P., ...

We report the discovery of an unusual low--ionization broad absorption line quasar at z=1.776 which exhibits absorption lines from many excited states of Feii. This member of the rare class of...

Observations of the Hubble Deep Field South with the Infrared Space Observatory - I. Observations, data reduction and mid-infrared source counts (2002)

Oliver, S., Mann, R. G., Carballo, R., Franceschini, A., Rowan-Robinson, M., Kontizas, M., ...

We present results from a deep mid-infrared survey of the Hubble Deep Field South (HDF-S) region performed at 7 and 15 micron with the CAM instrument on board the Infrared Space Observatory (ISO)....

Observations of the Hubble Deep Field South with the Infrared Space Observatory - II. Associations and star formation rates (2002)

Mann, R. G., Oliver, S., Carballo, R., Franceschini, A., Rowan-Robinson, M., Heavens, A. F., ...

We present results from a deep mid-IR survey of the Hubble Deep Field South (HDF-S) region performed at 7 and 15um with the CAM instrument on board ISO. We found reliable optical/near-IR associations...

Are galaxies shy ? (2002)

Elbaz, D.

Until 1996, there was little evidence that most galaxies were ``shy'', i.e. that they would hide their stars behind a veil of dust and turn red when forming stars, radiating the bulk of their...

The Bulk of the Cosmic Infrared Background Resolved by ISOCAM (2002)

Elbaz, D., Cesarsky, C., Chanial, P., Aussel, H., Franceschini, A., Fadda, D., ...

We have computed the 15 microns integrated galaxy light produced by ISOCAM galaxies above a sensitivity limit of 50 microJy. It sets a lower limit to the 15 microns extragalactic background light of...

A Long-Wavelength View on Galaxy Evolution from Deep Surveys by the Infrared Space Observatory (2001)

Franceschini, A., Aussel, H., Cesarsky, C. J., Elbaz, D., Fadda, D.

We discuss the constraints set on galaxy evolution by data from deep surveys performed in the mid-IR and far-IR with ISO and with mm telescopes at longer wavelengths. These reveal extremely high...

FIRBACK: III. Catalog, Source counts, and cosmological implications of the 170 micron ISO Deep survey (2001)

Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Bouchet, F. R., Cesarsky, C., ...

The FIRBACK (Far Infrared BACKground) survey is one of the deepest imaging surveys carried out at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of the structure of the Cosmic Far...

Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust Enshrouded Star Formation Rate (2001)

Chary, R., Elbaz, D.

We present a detailed interpretation of the spectrum of the cosmic infrared background longwards of 5 microns and of galaxy counts from various surveys at mid-infrared, far-infrared and submillimeter...

Ultimate sensitivity with ISOCAM (2000)

Altieri, B, Metcalfe, L, Blommaert, Joris; U0037630, Elbaz, D, Starck, JL, Aussel, H

We discuss the instrumental factors which constrain the sensitivity limits of the midinfrared camera (ISOCAM) of ESA's Infrared Space Observatory (ISO). The observing strategy judged to be best...

An excess of mid-IR luminous galaxies in Abell 1689? (2000)

Fadda, D., Elbaz, D., Flores, H., Franceschini, A., Cesarsky, C. J., ...

We present the results of infrared observations of Abell 1689 which was observed with ISOCAM, at 6.7\mic and 15\mic, and ISOPHOT at 200\mic. The cluster galaxies detected above a sensitivity limit of...

The European Large Area ISO Survey II: mid-infrared extragalactic source counts (2000)

Serjeant, S., Oliver, S., Rowan-Robinson, M., Crockett, H., Misoulis, V., Sumner, T., ...

We present preliminary source counts at 6.7um and 15um from the Preliminary Analysis of the European Large Area ISO survey, with limiting flux densities of \~2mJy at 15um & ~1mJy at 6.7um. We...

FIRBACK Source Counts and Cosmological Implications (2000)

Dole, Herve, Gispert, Richard, Lagache, Guilaine, Puget, Jean-Loup, Aussel, H., Bouchet, F. R., ...

FIRBACK is a one of the deepest surveys performed at 170 microns with ISOPHOT onboard ISO, and is aimed at the study of cosmic far infrared background sources. About 300 galaxies are detected in an...

The extragalactic background and its fluctuations in the far-infrared wavelengths (2000)

Lagache, G., Puget, J-L., Abergel, A., Bouchet, F. R., Boulanger, F., Ciliegi, P., ...

A Cosmic Far-InfraRed Background (CFIRB) has long been predicted that would traces the intial phases of galaxy formation. It has been first detected by Puget et al.(1996) using COBE data and has been...

Source Counts from the 15 microns ISOCAM Deep Surveys (1999)

Elbaz, D., Cesarsky, C. J., Fadda, D., Aussel, H., Desert, F. X., Franceschini, A., ...

We present the results of the five mid-IR 15 microns (12-18 microns LW3 band) ISOCAM Guaranteed Time Extragalactic Surveys performed in the regions of the Lockman Hole and Marano Field. The roughly...

An ISOCAM Mid-IR Survey through Gravitationally Lensing Galaxy Clusters (1999)

Biviano, A., Metcalfe, L., Altieri, B., Leech, K., Schulz, B., Kessler, M. F., ...

We present imaging results and source counts from a deep ISOCAM cosmological survey at 15 microns, through gravitationally lensing galaxy clusters. We take advantage of the cluster gravitational...

Isocam Extragalactic Mid-Infrared Deep Surveys Unveiling Dust-Enshrouded Star Formation In The Universe (1999)

Elbaz, D., Aussel, H., Cesarsky, C. J., Desert, F. X., Fadda, D., Franceschini, A., ...

ISOCAM extragalactic mid-infrared deep surveys have detected a population of strong IR emitters ten times more numerous than expected if there were no evolution from z

FIRBACK Far Infrared Survey with ISO: Data Reduction, Analysis and First Results (1999)

Dole, Herve, Lagache, Guilaine, Puget, Jean-Loup, Gispert, Richard, Aussel, H., Bouchet, F. R., ...

FIRBACK is one of the deepest cosmological surveys performed in the far infrared, using ISOPHOT. We describe this survey, its data reduction and analysis. We present the maps of fields at 175...

A Deep and Ultra-deep ISOCAM Cosmological Survey through Gravitationally Lensing Clusters of Galaxies (1999)

Metcalfe, L., Altieri, B., McBreen, B., Delaney, M., Biviano, A., ...

We present imaging results and source counts from an ISOCAM deep and ultra-deep cosmological survey through gravitationally lensing clusters of galaxies at 7 and 15 microns. A total area of about 53...

An ultra-deep ISOCAM observation through a cluster-lens (1999)

B. Altieri, L. Metcalfe, J. P. Kneib, B. Mcbreen, H. Aussel, A. Biviano, ...

. We present results of ultra-deep ISOCAM observations through a cluster-lens at 7¯m and 15¯m with the Infrared Space Observatory (ISO) satellite. These observations reveal a large number of...

FIRBACK: I. A deep survey at 175 $\mu$m with ISO, preliminary results (1998)

Puget, J. L., Lagache, G., Clements, D. L, Reach, W. T., Aussel, H., Bouchet, F. R, ...

FIRBACK is a deep survey conducted with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO) at an effective wavelength of 175 $\mu$m. We present here results we have obtained on the...

Medium-distant clusters of galaxies seen by ISO (1998)

Lemonon, L., Pierre, M., Cesarsky, C. J., Elbaz, D., Vigroux, L.

We present a comprehensive study of ISO cluster galaxies in connection with other wavelengths. First results show that infrared galaxies detected by ISOCAM concentrate on the edge of clusters....

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

An ultra-deep ISOCAM observation through a cluster-lens (1998)

Altieri, B., Metcalfe, L., Kneib, J. P., McBreen, B., Aussel, H., Biviano, A., ...

We present results of ultra-deep ISOCAM observations through a cluster-lens at 7 and 15 micron with the Infrared Space Observatory (ISO) satellite. These observations reveal a large number of...

ISOCAM observations of the Hubble Deep Field reduced with the PRETI method (1998)

Aussel, H., Cesarsky, C. J., Elbaz, D.

We have developed a new ISOCAM data reduction technique based on wavelet analysis, especially designed for the detection of faint sources in mid-infrared surveys. This method, the Pattern REcognition...

The FIRBACK 175 micron Survey (1998)

Clements, David L., Puget, J-L, Lagache, G., Dole, H., Cox, P., Gispert, R., ...

The FIRBACK project is a collaboration of eight institutes aimed at using long wavelength surveys with ISO to uncover the nature of the Cosmic Far-Infrared Background. We have surveyed nearly 4 sq....

Isocam deep surveys unveiling star formation in the mid-infrared (1998)

Elbaz, D., Aussel, H., Cesarsky, C. J., Desert, F. X., Fadda, D., Franceschini, A., ...

Before having exhausted the helium in its tank on April 8, 1998, the Infrared Space Observatory had time to perform several complementary surveys at various depths and areas within selected regions...

Deep ISOCAM view of the core of the lensing cluster A2390 (1998)

Lemonon, L., Pierre, M., Cesarsky, C. J., Elbaz, D., Pello, R., Soucail, G., ...

We have imaged the inner square arcminute of the well known lensing and cooling flow cluster A2390 (z = 0.23) down to a sensitivity of 65 and 130 microJy at 6.75 and 15 micronmetre, respectively. We...

ISO Mid-Infrared Observations of Abell 370 (1998)

Metcalfe, L., Altieri, B., Aussel, H., Biviano, A., Breen, B. Mc, Delaney, M., ...

We report on the mid-IR imaging at 7 and 10 microns of the galaxy cluster Abell 370, obtained with the ISOCAM instrument onboard ESA's Infrared Space Observatory (ISO), as part of an ongoing program...

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

Deep Galaxy survey at 6.75 micron with the ISO satellite (1998)

Flores, H., Hammer, F., Désert, F. X., Césarsky, C., Thuan, T., Crampton, D., ...

Deep 6.75um mid-IR ISOCAM observations were obtained of the Canada-France Redshift Survey (CFRS) 1415+52 field with the Infrared Space Observatory. The identification of the sources with optical...

Source Counts and Background Radiation (1997)

Franceschini, A., Aussel, H., Bressan, A., Cesarsky, C. J., Danese, L., De Zotti, G., ...

Our present understanding of the extragalactic source counts and background radiation at infrared and sub-mm wavelengths is reviewed. Available count data are used to constrain evolutionary models of...

First ISOCAM images of the Milky Way (1996)

Perault, M, Omont, A, Simon, G, Seguin, P, Ojha, D, Blommaert, Joris; U0037630, ...

ISOGAL is a 15 mu m ISOCAM survey of similar to 12 deg(2) in the Galactic Plane interior to \l\ = 45 degrees. In combination with IJK data from the near-infrared southern sky survey DENIS, the ISO...

ISOCAM mapping of the Whirlpool galaxy M 51 (1996)

Sauvage, M, Blommaert, Joris; U0037630, Boulanger, F, Cesarsky, CJ, Cesarsky, DA, Desert, FX, ...

We have obtained the first images of the 6.75 and 151 mu m continuum emission in the Whirlpool galaxy with ISOCAM, the infrared camera of the ISO1. These data reveal the well-developed, spiral arms...

Bimodal star formation in elliptical galaxies and the enrichment of the intra-cluster medium (1995)

Elbaz, D., Arnaud, M., Vangioni-Flam, E.

A detailed model of galactic evolution is proposed to explain both the iron content of the Intra-Cluster Medium (ICM) and of the ellipticals pertaining to the cluster. SNII are responsible for the...